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The high-energy gamma-ray emission of AP Librae
Univ Hamburg, Inst Experimentalphys, D-22761 Hamburg, Germany.
Max Planck Inst Kernphys, D-69029 Heidelberg, Germany ; Dublin Inst Adv Studies, Dublin 4, Ireland ; Natl Acad Sci Republ Armenia, Yerevan, Armenia .
Max Planck Inst Kernphys, D-69029 Heidelberg, Germany.
Natl Acad Sci Republ Armenia, Yerevan, Armenia ; Yerevan Phys Inst, Yerevan 375036, Armenia.
Vise andre og tillknytning
2015 (engelsk)Inngår i: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 573, artikkel-id A31Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The gamma-ray spectrum of the low-frequency-peaked BL Lac (LBL) object AP Librae is studied, following the discovery of very-high-energy (VHE; E > 100 GeV) gamma-ray emission up to the TeV range by the H.E.S.S. experiment. Thismakes AP Librae one of the few VHE emitters of the LBL type. The measured spectrum yields a flux of (8.8 +/- 1.5(stat) +/- 1.8(sys)) x 10(-12) cm(-2) s(-1) above 130 GeV and a spectral index of Gamma = 2.65 +/- 0.19(stat) +/- 0.20(sys). This study also makes use of Fermi-LAT observations in the high energy (HE, E > 100 MeV) range, providing the longest continuous light curve (5 years) ever published on this source. The source underwent a flaring event between MJD 56 306-56 376 in the HE range, with a flux increase of a factor of 3.5 in the 14 day bin light curve and no significant variation in spectral shape with respect to the low-flux state. While the H.E.S.S. and (low state) Fermi-LAT fluxes are in good agreement where they overlap, a spectral curvature between the steep VHE spectrum and the Fermi-LAT spectrum is observed. The maximum of the gamma-ray emission in the spectral energy distribution is located below the GeV energy range.

sted, utgiver, år, opplag, sider
2015. Vol. 573, artikkel-id A31
Emneord [en]
galaxies: active, BL Lacertae objects: individual: AP Librae, gamma rays: galaxies
HSV kategori
Forskningsprogram
Fysik, Astropartikelfysik
Identifikatorer
URN: urn:nbn:se:lnu:diva-40902DOI: 10.1051/0004-6361/201321436ISI: 000346901300001Scopus ID: 2-s2.0-84936998181OAI: oai:DiVA.org:lnu-40902DiVA, id: diva2:795876
Tilgjengelig fra: 2015-03-17 Laget: 2015-03-17 Sist oppdatert: 2019-02-14bibliografisk kontrollert

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